Table 1
Flow parameters of H, D, and He at TS used in the simulations.
| Population | λ [°] | φ [°] | T [K] | V [km s-1] | n0 [cm-3] |
|
|
|||||
Primary |
255.4 | 5.31 | 6020 | 28.512 | 0.0312(2) |
| Secondary |
255.4 | 5.31 | 16300 | 18.744 | 0.0542(2) |
NISHe |
259.2 | 5.12 | 6165 | 22.756 | 0.0150(4) |
Notes.The densities of the primary and secondary populations are listed for H, the density labeled as NIS He population is for He. The densities of D populations were adopted as for H, multiplied by the interstellar abundance ξNISD = 15.6 ppm (see text). The density of O at TS was adopted 5 × 10-3 cm-3 after Slavin & Frisch (2007).
Reference. (1) Izmodenov et al. (2003); (2) Bzowski et al. (2008); (3) Bzowski et al. (2012); (4) Witte (2004).
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